LERMA UMR8112

Laboratoire d’Études du Rayonnement et de la Matière en Astrophysique et Atmosphères



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Address and access to LERMA sites

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LERMA is situated on 5 sites in the Paris region:

- Observatoire de Paris (Paris and Meudon sites)
- University Pierre and Marie Curie (UPMC)
- ENS
- University of Cergy Pontoise (UCP)

Access to Observatoire de Paris (Paris site)
- Postal Address : 61, avenue de l’Observatoire - 75014 PARIS
- Pedestrian and vehicle access: 77, Avenue Denfert-Rochereau - 75014 Paris
- Telephone: +33 1 40 51 22 21 - Fax : +33 1 43 54 18 04
- Access

Access to Observatoire de Paris (Meudon site)
- Postal address and pedestrian access: Observatoire de Paris, site de Meudon - 5, place Jules Janssen - 92195 Meudon cedex
- Vehicle access and goods: 11, avenue Marcelin Berthelot, 92195 Meudon
- Standard : +33 1 45 07 75 30
- Access

Access to UPMC
- Postal address : UPMC - case courrier 76 - 4 place Jussieu - 75252 Paris cedex 05
- Pedestrian access : 4, place Jussieu - 75252 Paris cedex 05
- Access :

  • Tour 32-33 2ème et 3ème étage
  • Tour 24-34 5ème étage

Access to l’ENS
- Postal address : LERMA/L.R.A. - Département de Physique ENS - 24, rue Lhomond - 75231 PARIS Cedex 05
- Accès

Access to Cergy Pontoise
- Postal address : LERMA/LAMAP - Site de Neuville II - UFR Sciences et Techniques - Département de physique - 5, mail Gay Lussac - 95031 Cergy-Pontoise cedex
- Access

Séminaires à venir

Vendredi 12 juin 2020, 14h00
,
visioconférence
Observational and theoretical constraints on the formation and early evolution of the first dust grains in galaxies at 5 < z < 10
Denis BURGARELLA
Laboratoire d'Astrophysique de Marseille
résumé :
The first generation of stars were born a few hundred million years after the big bang. These stars synthesized elements heavier than H and He, that are later expelled into the interstellar medium, initiating the rise of metals. Within this enriched medium, the first dust grains formed. This event is cosmological crucial for molecule formation as dust plays a major role by cooling low-metallicity star-forming clouds which can fragment to create lower mass stars. Collecting information on these first dust grains is difficult because of the negative alliance of large distances and low dust masses. We combine the observational information from galaxies at redshifts 5 < z < 10 to constrain their dust emission and theoretically understand the first evolutionary phases of the dust cycle. Spectral energy distributions (SEDs) are fitted with CIGALE and the physical parameters and their evolution are modelled. From this SED fitting, we build a dust emission template for this population of galaxies in the epoch of reionization. Our new models explain why some early galaxies are observed and others are not. We follow in time the formation of the first grains by supernovae later destroyed by other supernova blasts and expelled in the circumgalactic and intergalactic media.
 
Vendredi 3 juillet 2020, 14h00
,
visioconférence
Tba
Patricia TISSERA
Universidad Andres Bello, Santiago
résumé :
Tba
 
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